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Coalescing compact binaries of neutron stars and/or black holes areconsidered as one of the most promising sources for Earth based gravitationalwave detectors. The LIGO-Virgo joint collaboration's Compact Binary Coalescence(CBC) group is searching for gravitational waves emitted by these astrophysicalsystems by matched filtering the data against theoretically modeled templatewaveforms. A variety of waveform template families are employed depending onthe mass range probed by the search and the stage of the inspiral phasetargeted: restricted post-Newtonian for systems having total mass less than $35\msun$, numerical relativity inspired complete inspiral-merger-ringdownwaveforms for more massive systems up to $100\msun$ and ringdown templates formodeling perturbed black holes up to $500\msun$. We give a status update on CBCgroup's current efforts and upcoming plans in detecting signatures ofastrophysical gravitational waves.

LIGO-Virgo searches for gravitational waves from coalescing binaries: a status update